Physics · nuclei · NEET
No. Half-life is a fixed property of the nucleus. Whether you start with 1000 atoms or 1 crore atoms, exactly half decay in one half-life. A bigger sample decays MORE atoms per second (higher activity), but the TIME to lose half stays the same. This is because decay is a fraction-based (exponential) process, not a fixed number per second.
No, this is the most common mistake. After 1 half-life, half is left (1/2). After 2 half-lives, half of that half is left, so 1/4 remains, not zero. Half-lives do not add up to finish the sample. Fraction left after n half-lives = (1/2) to the power n. The sample never fully reaches zero in theory.
No. Mean life (tau) is the AVERAGE life of all nuclei and is longer than half-life. The link is tau = 1/lambda and T = 0.693/lambda, so T = 0.693 x tau, meaning half-life is about 69.3 percent of mean life. Half-life = time for half to go; mean life = average survival time.
It is ln 2 (natural log of 2). Start from the decay law N = N0 e^(-lambda t). At one half-life, N = N0/2. So 1/2 = e^(-lambda T). Taking natural log: ln(1/2) = -lambda T, which gives lambda T = ln 2 = 0.693. So T = 0.693/lambda. The 2 appears because we are halving.
No. Radioactive decay comes from inside the nucleus, so it is not affected by outside conditions like heat, pressure, or whether the atom is in a compound. Half-life stays constant for a given isotope. This makes it useful for carbon dating and finding the age of rocks.
T = 0.693 / lambda, where lambda is the decay constant. Also T = 0.693 x tau, where tau is the mean life.
The second (s). In practice half-lives are quoted in seconds, minutes, days, or years depending on the isotope.
Fraction left = (1/2)^3 = 1/8, which is 12.5 percent. The rest (7/8) has decayed.
Yes, inversely. A larger decay constant lambda means a shorter half-life (faster decay), since T = 0.693/lambda.
No. Each isotope has its own fixed half-life, ranging from tiny fractions of a second to billions of years (for example, uranium-238 has a half-life of about 4.5 billion years).